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相关论文: NuSTAR observations of water megamaser AGN

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Recently, Papadopoulos et al., 2010 using sub-mm CO molecular line observations of nearby ultra-luminous IRAS galaxies, (U)LIRGs, have found that exceptionally large gas column densities (N_H > 10^25 cm-2) can be present across some of the…

宇宙学与河外天体物理 · 物理学 2015-05-19 I. Georgantopoulos , E. Rovilos , A. Akylas , E. Xilouris

We present \nustar{} observation of the atoll type neutron star (NS) low-mass X-ray binary (LMXB) Serpens~X-1 (Ser~X-1) performed on 17 February 2018. We observed Ser~X-1 in a soft X-ray spectral state with 3-79 keV luminosity of…

高能天体物理现象 · 物理学 2020-05-06 Aditya S. Mondal , Gulab C. Dewangan , B. Raychaudhuri

We assume that dust near active galactic nuclei (AGN) is distributed in a torus-like geometry, which may be described by a clumpy medium or a homogeneous disk or as a combination of the two (i.e. a 2-phase medium). The dust particles…

星系天体物理 · 物理学 2015-11-11 Ralf Siebenmorgen , Frank Heymann , Andreas Efstathiou

We present polarimetric maps of the Circinus galaxy nucleus in the $BVRI$ bands, obtained with VLT/FORS2. Circinus is the closest Seyfert 2 galaxy and harbours an archetypal obscured active galactic nucleus (AGN). Recent high angular…

We report on an observation of the neutron star low-mass X-ray binary Serpens X-1, made with NuSTAR. The extraordinary sensitivity afforded by NuSTAR facilitated the detection of a clear, robust, relativistic Fe K emission line from the…

In Unification Models, Active Galactic Nuclei (AGN) are believed to be surrounded by an axisymmetric structure of dust and gas, which greatly influences their observed properties according to the direction from which they are observed. The…

天体物理学 · 物理学 2009-11-11 E. Ibar , P. Lira

We present results from a coordinated $XMM$-$Newton$+$NuSTAR$ observation of the type 1.8 Seyfert galaxy IRAS 13197-1627. This is a highly complex source, with strong contributions from relativistic reflection from the inner accretion disk,…

高能天体物理现象 · 物理学 2017-12-06 D. J. Walton , M. Brightman , G. Risaliti , A. C. Fabian , F. Fuerst , F. A. Harrison , A. Lohfink , G. Matt , G. Miniutti , M. L. Parker , D. Stern

We present observations of the molecular gas in the nuclear environment of three prototypical low luminosity AGN (LLAGN), based on VLT/SINFONI AO-assisted integral-field spectroscopy of H2 1-0 S(1) emission at angular resolutions of ~0.17".…

宇宙学与河外天体物理 · 物理学 2015-06-12 F. Müller-Sánchez , M. A. Prieto , M. Mezcua , R. I. Davies , M. Malkan , M. Elitzur

Context. The putative tori surrounding the accretion disks of active galactic nuclei (AGNs) play a fundamental role in the unification scheme of AGNs. Infrared long-baseline interferometry allows us to study the inner dust distribution in…

Emission from high-J CO lines in galaxies has long been proposed as a tracer of X-ray dominated regions (XDRs) produced by AGN. Of particular interest is the question of whether the obscuring torus, which is required by AGN unification…

We present results from a deep, coordinated $XMM$-$Newton$+$NuSTAR$ observation of the Seyfert 2 galaxy IRAS 00521-7054. The $NuSTAR$ data provide the first detection of this source in high-energy X-rays ($E > 10$ keV), and the broadband…

高能天体物理现象 · 物理学 2019-01-23 D. J. Walton , E. Nardini , L. C. Gallo , M. T. Reynolds , C. Ricci , T. Dauser , A. C. Fabian , J. A. Garcia , F. A. Harrison , G. Risaliti , D. Stern

In a sample of local active galactic nuclei studied at a spatial resolution on the order of 10 pc we show that the interstellar medium traced by the molecular hydrogen v=1-0 S(1) 2.1um line forms a geometrically thick, clumpy disk. The…

星系天体物理 · 物理学 2011-02-11 E. K. S. Hicks , R. I. Davies , M. A. Malkan , R. Genzel , L. J. Tacconi , F. Muller Sanchez , A. Sternberg

We present a detailed study of the X-ray and optical spectra of the luminous Seyfert galaxy Mrk 1393, which revealed variable partial obscuration of the active nucleus. The X-ray spectra obtained by XMM-Newton and Swift show moderate…

宇宙学与河外天体物理 · 物理学 2009-11-13 T. G. Wang , H. Y. Zhou , D. Grupe , W. M. Yuan , X. B. Dong , H. L. Lu

For the first time in an extragalactic source, we detect linearly polarized water maser emission associated with the molecular accretion disk of NGC 1068. The position angles of the electric polarization vectors are perpendicular to the…

We have analyzed the broadband X-ray spectra of active galactic nuclei (AGNs) in two "non-merging" luminous infrared galaxies (LIRGs) UGC 2608 and NGC 5135, utilizing the data of NuSTAR, Suzaku, XMM-Newton, and Chandra. Applying the X-ray…

高能天体物理现象 · 物理学 2020-07-15 Satoshi Yamada , Yoshihiro Ueda , Atsushi Tanimoto , Saeko Oda , Masatoshi Imanishi , Yoshiki Toba , Claudio Ricci

Recently, a relationship between the water maser detection rate and far infrared (FIR) flux density has been found as a result of a 22 GHz maser survey in a sample comprised of northern galaxies with 100 micron flux density > 50 Jy and a…

天体物理学 · 物理学 2007-12-06 P. Castangia , A. Tarchi , C. Henkel , K. M. Menten

Advancements in infrared IR open up the possibility to spatially resolve AGN on the parsec-scale level and study the circumnuclear dust distribution, commonly referred to as the "dust torus", that is held responsible for the type 1/type 2…

We report the discovery of water maser emission in five active galactic nuclei (AGN) with the 100-m Green Bank Telescope (GBT). The positions of the newly discovered masers, measured with the VLA, are consistent with the optical positions…

天体物理学 · 物理学 2008-11-26 Paul T. Kondratko , Lincoln J. Greenhill , James M. Moran

New Gemini mid-infrared spectroscopic observations together with Spitzer Space telescope archival data, are used to study the properties of the dusty torus and circumnuclear star formation in the active galaxies NGC 7213 and NGC 1386. Our…

星系天体物理 · 物理学 2015-06-18 Daniel Ruschel-Dutra , Miriani Pastoriza , Rogério Riffel , Dinalva A. Sales , Cláudia Winge

NGC7538 is a complex massive star-forming region. The region is composed of several radio continuum sources, one of which is IRS1, a high-mass protostar, from which a 0.3 pc molecular bipolar outflow was detected. Several maser species have…

太阳与恒星天体物理 · 物理学 2015-05-28 G. Surcis , W. H. T. Vlemmings , R. M. Torres , H. J. van Langevelde , B. Hutawarakorn Kramer
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